Search Results - "Noda, Tsuneo"

Effects of Nuclear Equation of State on Type-I X-ray Bursts and Implication for Clocked Burster GS 1826–24 by Dohi, Akira, Nishimura, Nobuya, Hashimoto, Masa-aki, Matsuo, Yasuhide, Noda, Tsuneo, Nagataki, Shigehiro

“…We study the effects of nuclear equation of state (EOS) on Type-I X-ray bursts, focusing on the Clocked burster GS 1826–24. According to the shell-flush model,…”
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Guideline for Gynecological Practice in Japan: Japan Society of Obstetrics and Gynecology and Japan Association of Obstetricians and Gynecologists 2020 edition by Kawaguchi, Ryuji, Matsumoto, Koji, Ishikawa, Tetsuya, Ishitani, Ken, Okagaki, Ryugo, Ogawa, Mariko, Oki, Toshimichi, Ozawa, Nobuaki, Kawasaki, Kaoru, Kuwabara, Yoshimitsu, Koga, Kaori, Sato, Yuichi, Takai, Yasushi, Tanaka, Kyoko, Tanebe, Kyoko, Terauchi, Masakazu, Todo, Yukiharu, Nose‐Ogura, Sayaka, Noda, Tsuneo, Baba, Tsukasa, Fujii, Eriko, Fujii, Takuma, Miyazaki, Hiroaki, Yoshino, Osamu, Yoshimura, Kazuaki, Maeda, Tsugio, Kudo, Yoshiki, Kobayashi, Hiroshi

“…Nine years after the first edition of The Guideline for Gynecological Practice, which was jointly edited by The Japan Society of Obstetrics and Gynecology and…”
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Cooling of neutron stars with quark-hadron continuity by Noda, Tsuneo, Yasutake, Nobutoshi, Hashimoto, Masa-aki, Maruyama, Toshiki, Tatsumi, Toshitaka

“…Neutron stars are high-density objects formed by the gravitational collapse of massive stars, and the whole star can be likened to a giant nucleus. The…”
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Quiescent Light Curve of Accreting Neutron Star MAXI J0556-332 by Liu, Helei, Matsuo, Yasuhide, Hashimoto, Masa-aki, Noda, Tsuneo, Fujimoto, Masayuki Y.

“…MAXI J0556-332 is the hottest transient accreting neutron star at the beginning of its quiescence. A theoretical model with crustal heating indicates that an…”
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Palliative care needs of cancer outpatients receiving chemotherapy: an audit of a clinical screening project by Morita, Tatsuya, Fujimoto, Koji, Namba, Miki, Sasaki, Naoko, Ito, Tomoko, Yamada, Chika, Ohba, Arisa, Hiroyoshi, Motoki, Niwa, Hiroshi, Yamada, Takeshi, Noda, Tsuneo

“…Purpose Although more and more cancer patients are receiving chemotherapy in outpatient settings in their advanced stage and could have a broad range of…”
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COOLING OF COMPACT STARS WITH COLOR SUPERCONDUCTING PHASE IN QUARK-HADRON MIXED PHASE by Noda, Tsuneo, Hashimoto, Masa-aki, Yasutake, Nobutoshi, Maruyama, Toshiki, Tatsumi, Toshitaka, Fujimoto, Masayuki

“…We present a new scenario for the cooling of compact stars considering the central source of Cassiopeia A (Cas A). The Cas A observation shows that the central…”
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Possibility of rapid neutron star cooling with a realistic equation of state by Dohi, Akira, Nakazato, Ken’ichiro, Hashimoto, Masa-aki, Yasuhide, Matsuo, Noda, Tsuneo

“…Abstract Whether fast cooling processes occur or not is crucial for the thermal evolution of neutron stars. In particular, the threshold of the direct Urca…”
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Thermal state of transiently accreting neutron stars with additional heating beyond deep crustal heating by Liu, Helei, Hashimoto, Masa-aki, Lü, Guoliang, Matsuo, Yasuhide, Wen, Dehua, Noda, Tsuneo

“…Abstract As some neutron star transients require an additional unknown heat source (referred to as “shallow heating”) to explain their high temperatures at the…”
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Constraints on the Neutron-Star Structure from the Clocked X-Ray Burster 1RXS J180408.9$-$342058 by Dohi, Akira, Iwakiri, Wataru, Nishimura, Nobuya, Noda, Tsuneo, Nagataki, Shigehiro, Hashimoto, Masa-aki

“…Type-I X-ray bursts are rapid-brightening transient phenomena on the surfaces of accreting neutron stars (NSs). Some X-ray bursts, called {\it clocked…”
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Cooling of Isolated Neutron Stars with Pion Condensation: Possible Fast Cooling in a Low-Symmetry-Energy Model by Dohi, Akira, Liu, Helei, Noda, Tsuneo, Hashimoto, Masa-aki

“…We studied thermal evolution of isolated neutron stars (NSs) including the pion condensation core, with an emphasis on the stiffness of equation of state…”
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Impacts of the direct URCA and Superfluidity inside a Neutron Star on Type-I X-Ray Bursts and X-Ray Superbursts by Dohi, Akira, Nishimura, Nobuya, Sotani, Hajime, Noda, Tsuneo, Liu, Helei, Nagataki, Shigehiro, Hashimoto, Masa-aki

“…ApJ 937 124 (2022) We investigate the impacts of neutrino cooling mechanism inside the neutron star (NS) core on the light curves of type-I X-ray bursts and…”
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Quiescent luminosities of accreting neutron stars with different equation of states by Liu, Helei, Dohi, Akira, Hashimoto, Masa-aki, Matsuo, Yasuhide, Lü, Guo-Liang, Noda, Tsuneo

“…We model the quiescent luminosity of accreting neutron stars with several equation of states (EOSs), including the effect of pion condensation and…”
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Possibility of rapid neutron star cooling with the realistic equation of state by Dohi, Akira, Nakazato, Ken'ichiro, Hashimoto, Masa-aki, Matsuo, Yasuhide, Noda, Tsuneo

“…Prog.Theor.Exp.Phys.2019,113E01 Whether fast cooling processes occur or not is crucial for the thermal evolution of neutron stars. In particular, the threshold…”
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Utility of predeposit autologous blood donation by switch back method combined with recombinant human erythropoietin in gynecological surgery by Itani, Y, Ito, K, Hori, K, Tamori, N, Adachi, S

“…To apply recombinant human (rh)erythropoietin (EPO) to predeposit autologous blood donation (P.A.B.D.) in cancer patients clinically, (1) we tested the effects…”
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Quiescent Light Curve of Accreting Neutron Star MAXI J0556-332 by Liu, Helei, Matsuo, Yasuhide, Hashimoto, Masa-aki, Noda, Tsuneo, Fujimoto, Masayuki Y

“…MAXI J0556-332 is the hottest transient accreting neutron star at the beginning of its quiescence. A theoretical model with crustal heating indicates that an…”
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Thermal structures of accreting neutron stars with neutrino losses due to strong pion condensations by Matsuo, Yasuhide, Hashimoto, Masa-aki, Hayashida, Koutarou, Liu, Helei, Noda, Tsuneo, Fujimoto, Masayuki Y

“…Quiescent X-ray luminosities are presented in low mass X-ray binaries with use of evolutionary calculations. The calculated luminosities are compared with…”
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Cooling of Compact Stars with Color Superconducting Quark Matter by Noda, Tsuneo, Yasutake, Nobutoshi, Hashimoto, Masa-aki, Maruyama, Toshiki, Tatsumi, Toshitaka, Fujimoto, Masayuki Y

“…We show a scenario for the cooling of compact stars considering the central source of Cassiopeia A (Cas A). The Cas A observation shows that the central source…”
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Thermodynamical description of hadron-quark phase transition and its implications on compact-star phenomena by Yasutake, Nobutoshi, Noda, Tsuneo, Sotani, Hajime, Maruyama, Toshiki, Tatsumi, Toshitaka

“…Nova, (2013), Chap.4, pp.63, ISBN 9781622579709 One of the most promising possibilities may be the appearance of quark matter in astrophysical phenomena in the…”
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Cooling of Compact Stars with Color Superconducting Phase in Quark Hadron Mixed Phase by Noda, Tsuneo, Hashimoto, Masa-aki, Yasutake, Nobutoshi, Maruyama, Toshiki, Tatsumi, Toshitaka, Fujimoto, Masayuki Y

“…2012, ApJ, 765, 1 We present a new scenario for the cooling of compact stars considering the central source of Cassiopeia A (Cas A). The Cas A observation…”
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Prognostic results of cisplatin IP and carboplatin IV with G-CSF in patients with ovarian cancer by Adachi, S, Itani, Y, Ito, K, Noda, T, Shintani, M, Saito, K, Furukawa, N, Tomii, Y

“…We performed a dose-escalation study of carboplatin combined with a fixed dose of intraperitoneal cisplatin and G-CSF in patients with epithelial ovarian…”
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